1 / 21

Bernhard Holzer

”Beam Dynamics for Nb3Sn dipoles ... latest news". Bernhard Holzer. IP5. IR 7. IP8. IP1. IP2. *. DS Upgrade Scenarios. halo. Shift 12 Cryo -magnets, DFB, and connection cryostat in each DS. transversely shifted by 4.5 cm. halo. New ~3..3.5 m shorter Nb 3 Sn Dipoles (2 per DS).

sanjiv
Download Presentation

Bernhard Holzer

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. ”Beam Dynamics for Nb3Sn dipoles ... latest news" Bernhard Holzer IP5 IR 7 IP8 IP1 IP2 *

  2. DS Upgrade Scenarios halo Shift 12 Cryo-magnets, DFB, and connection cryostat in each DS transversely shifted by 4.5 cm halo New ~3..3.5 m shorter Nb3Sn Dipoles (2 per DS) -4.5m shifted in s +4.5 m shifted in s M. Karppinen TE-MSC-ML

  3. Effects to be expected: * magnets are shorter than MB Standards change of geometry distortion of design orbit * R-Bends  S-Bends  edge focusing distortion of the optics tune shift, beta beat * nonlinar transfer function (3.5 TeV)  distortion of closed orbit to be corrected locally ?? dedicated corrector coils ?? trim power supply ?? * feed down effects from sagitta ? * multipole effect on dynamic aperture ? Sixtrack Tracking Simulations

  4. The persistent current problem: Very First Multipole Estimates tracking studies & prototype measurements needed b3 remanence as a function of precycle (pre-injection plateau) B.Auchmann Comparison: b3 Hysteresis Nb3Sn / NbTi M. Karppinen

  5. Nb3Sn Dipole: Multipole Errors, “Pure Estimation !!” ... in the usual units, i.e. 10 -4 referred to the usual ref radius = 17mm

  6. Nb3Sn Dipole: Multipole Errors, “Pure Estimation !!”

  7. NbTi Dipole: Multipole Errors:

  8. Where are we ? IP1,2,5,IP7 Q8 Q9 Q10 Present Option: 2 x 5.5m Nb3Sn Dipoles separated

  9. optics situation collision optics, 7 TeV no big difference in optical functions between injection / luminosity

  10. Tracking Studies: Dynamic Aperture determined via stability / survival time theory: phase space ellipse defined by optical parameters ideal, linear machine strong b3 multipole Phase Space Distance b3 = 98, full & local correction b3 = 98, no correction

  11. Tracking Studies: Dynamic Aperture determined via survival time b3 = 98, no correction survival time ... measured in number of turns ... gives an indication of the influence of the non-linear fields on the ( an- ) harmonic oscillation of the particles. y For the experts: 60 seeds, 10^5 turns, 4-18 σ in units of 2, 30 particle pairs, 17 angles x

  12. Field Quality: Dynamic Aperture Studies 7 TeV Case, luminosity optics (55cm) ε=5*10-10 radm ( εn= 3.75μm) ideal Nb3Sn dipoles mult. coeff. à la error table6 at high field the higher harmonics are small enough, the p.c. effects disappeared and the emittance is reduced (Liouville)

  13. Field Quality: Dynamic Aperture Studies injection optics, 450 GeV, influence of b3 values, 2 IP’s = 8 dipoles dyn aperture injection optics, minimum of 60 seeds dynamic aperture for Nb3Sn full error table (blue) b3 = 0 an = bn = 0 the first estimated errors lead to extreme reduction in dyn. aperture main problem: b3

  14. Field Quality: Dynamic Aperture Studies Injection Optics, 450 GeV, Scan of b3 dyn aperture injection optics, minimum of 60 seeds dynamic aperture for Nb3Sn case: full error table (red) b3 reduced to 50% (green) b3 reduced to 25% (violett) b3 = 0 and to compare with: present LHC injection for the experts: unlike to the collision case: at injection the b3 of the Nb3Sn dipoles is the driving force to the limit in dynamic aperture. A scan in b3 values has been performed and shows that values up to b3 ≈ 20 units are ok.

  15. Field Quality: Dynamic Aperture Studies Injection Optics, 450 GeV, Different Sectors dyn aperture for Nb3Sn dipoles in #2,7 and in #1,2,5 standard spool piece correctors optimised for Q’ correction per octant #2,7, an=bn=0 #2,7 b3=27 #1,2,5 b3=27 #2,7 first estimate, “error table 2”

  16. Field Quality: Dynamic Aperture Studies Injection Optics, 450 GeV, ATS dyn aperture for Nb3Sn dipoles #1,2,5 ATS shows a increased sensitivity for higher multipoles, -> tighter limit for b3 and higher an / bn ATS Lattice #1,2,5 an=bn=0 #1,2,5 b3=0 #1,2,5 bn=20 #1,2,5 b3=27

  17. Field Quality: Dynamic Aperture Studies Injection Optics, 450 GeV, first measured values: “FNAL-demo-2” measured values for the “systematics” FNAL best guess for the ramndom errors Mikko et al

  18. Field Quality: Dynamic Aperture Studies Injection Optics, 450 GeV, first measured values: “FNAL-demo-2” and again the tracking ... systematics -> FNAL prototype random -> best guess uncertainty - > MB standard dipole ideal Nb3Sn dipoles, an=bn=0 first FNAL prototype systematics & Mikkos random artificially enhanced b4...6 , a3 first measured values are just at the limit but at the moment in sufficient dynamic aperture is obtained.

  19. Preliminary (!) Resumée: first estimates / calculations for pc systematics ... where chilling limits calculated for higher multipole coefficients (mainly b3) first measurement results are “just within” these limits problem: injection energy / optics large emittance, large p.c. effects ATS injection / luminosity seems a bit more sensitive than LHC standard optics unknown: realistic values for random errors ? do we have to deal with uncertainties ? limits for individual higher coefficients Plan & Next Steps: follow up closely the new results

  20. ParticleTrackingCalculations particlevector: field at particleposition Idea: calculatetheparticlecoordiantes x, x´ throughthe linear lattice … usingthematrixformalism. ifyouencounter a nonlinearelement (e.g. sextupole): stop calculateexplicitlythemagneticfield at theparticlescoordinate calculate kick on the particle and continue with the linear matrix transformations

More Related